2006ApJ...648L.139T


Query : 2006ApJ...648L.139T

2006ApJ...648L.139T - Astrophys. J., 648, L139-L142 (2006/September-2)

Cyclotron resonance energies at a low X-ray luminosity: A0535+262 observed with Suzaku.

TERADA Y., MIHARA T., NAKAJIMA M., SUZUKI M., ISOBE N., MAKISHIMA K., TAKAHASHI H., ENOTO T., KOKUBUN M., KITAGUCHI T., NAIK S., DOTANI T., NAGASE F., TANAKA T., WATANABE S., KITAMOTO S., SUDOH K., YOSHIDA A., NAKAGAWA Y., SUGITA S., KOHMURA T., KOTANI T., YONETOKU D., ANGELINI L., COTTAM J., MUKAI K., KELLEY R., SOONG Y., BAUTZ M., KISSEL S. and DOTY J.

Abstract (from CDS):

The binary X-ray pulsar A0535+262 was observed with the Suzaku X-ray observatory on 2005 September 14 for a net exposure of 22 ks. The source was in the declining phase of a minor outburst, exhibiting 3-50 keV luminosity of ∼3.7x1035 ergs/s at an assumed distance of 2 kpc. In spite of the very low source intensity (about 30 mcrab at 20 keV), its electron cyclotron resonance was detected clearly with the Suzaku Hard X-Ray Detector, in absorption at about 45 keV. The resonance energy is found to be essentially the same as that measured when the source is almost 2 orders of magnitude more luminous. These results are compared with the luminosity-dependent changes in the cyclotron resonance energy, observed from 4U 0115+63 and X0331+53.

Abstract Copyright: ∼

Journal keyword(s): Magnetic Fields - Stars: Pulsars: Individual: Alphanumeric: A0535+26 - Stars: Neutron - X-Rays: Binaries

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* V635 Cas HXB 01 18 31.9704955824 +63 44 33.072603144 17.05 16.64 15.19 14.34 13.22 B0.2Ve 791 0
2 V* BQ Cam HXB 03 34 59.9116110096 +53 10 23.296879776   17.16 15.42 14.26 13.04 O8.5Ve 525 1
3 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
4 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
5 HD 245770 HXB 05 38 54.5748918624 +26 18 56.836952784 9.30 9.84 9.39 8.77 8.30 O9/B0III/Ve 1045 0

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